POSSIBLE
SMC
|
| LHA 115-N 55 | IRAS F00535-7219 | GSC2.4.2 S0WB245329 | AAVSO - |
| SIMBAD LHA 115-N 55 | Pan-STARRS - | SAO - | VSX - |
| GAIA DR3 4689070750646585472 | SkyMapper 005517.55-720310.8 | WRAY - | GCVS - |
| 2MASS J00551754-7203109 | HIP - | Hen - | BD - |
| WISE J005517.55-720310.8 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 13.8231Ref | Parallax (mas) | -0.056±0.027Ref | Reddening E(B-V) (mag) | 0.15±0.02Ref, Note |
| Declination (°) | -72.0530Ref | Distance (kpc) | 62.1±1.9Ref 19.69Ref, Note, 27.26Ref, Note |
||
| Galactic longitude (°) | 302.5115Ref | Proper motion in α (mas/yr) | 0.78±0.03Ref | ||
| Galactic latitude (°) | -45.0721Ref | Proper motion in δ (mas/yr) | -1.30±0.03Ref |
| X-Ray | NoRef | IR type | D?Ref | Radio | - |
| X-Ray type | - | J (mag) | 14.24Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 13.63Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 12.64Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 10.35Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 8.82Ref | Resolved nebula | - |
| U (mag) | 15.85Ref | WISE W3 (mag) | 6.02Ref | IPmax (eV) | 99Ref |
| B (mag) | 16.14Ref | WISE W4 (mag) | 4.56Ref | [O III] lines | YesRef |
| V (mag) | 15.61Ref | IRAS 12μm (Jy) | 0.15Ref | He II lines | YesRef |
| R (mag) | - | IRAS 25μm (Jy) | 0.12Ref | [Fe VII] lines | Yes?Ref |
| I (mag) | 14.82Ref | IRAS 60μm (Jy) | 0.82Ref | O VI lines | NoRef |
| BP (mag) | 15.49Ref | IRAS 100μm (Jy) | 5.28Ref | ||
| G (mag) | 15.18Ref | AKARI S09 (Jy) | 0.13Ref | ||
| RP (mag) | 14.58Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | - | Size of giant’s orbit (AU) | - |
| Eccentricity | - | RV of giant (km/h) | - | Separation (AU) | - |
| Inclination (°) | - | Inferior conj. of giant (JD) | - | Mass function | - |
| Eclipses | - | Mass ratio | - | ||
| Orbital ephemeris | - |
| Spectral type | - | Mass (M⊙) | - | Pulsation | YesRef |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | D?Ref | Luminosity (L⊙) | - | Pulsation period (days) | 147.37Ref |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | - | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Included in the list of possible symbiotic stars or closely related objects in Munari & Zwitter (2002), this star's spectrum shows many emission lines. It has been classified as a planetary nebula (PN) by Lindsay (1961), a VV Cep star by Walker (1983), and an extreme AGB star in Boyer et al. (2011). The star exhibits variability with a period of 147 days and long-term sinusoidal variability, as reported in Soszyński et al. (2011).